Tunable ferro-electric filter

ABSTRACT

The present invention quantifies and reduces losses in tunable bandpass filters having ferro-electric capacitors. Given a required insertion loss and the quality factor of a resonator, the geometric losses resulting from a particular topology for the ferro-electric capacitor and the metal losses are accounted for to quantify the allowable ferro-electric losses.

RELATED APPLICATION

This Application is a continuation of U.S. patent application Ser. No. 09/904,631, filed Jul. 13, 2001, and entitled “Tunable Ferro-Electric Filter”, now U.S. Pat. No. 6,690,251. This application also claims the benefit of U.S. Provisional Application No. 60/283,093, filed Apr. 11, 2001, and entitled “Low Loss Tunable Ferro-Electric Device and Method of Characterization”, which is hereby incorporated by reference.

BACKGROUND Description of Related Art

Filters, such as bandpass filters, have numerous applications in communications and electronics. For example, in wireless communications a given frequency band must accommodate many wireless users. To accommodate so many users, stringent bandpass filtering requirements must be achieved because of the crowded frequency allocations provided.

At present, wireless handsets use fixed-tuned bandpass filters (BPFs) to meet their filtering specifications. The design of such filters is complicated because they must achieve the lowest possible passband insertion loss (I.L.) while simultaneously achieving a specified large out-of-band rejection. As a specific example, consider full band PCS CDMA handsets using fixed bandwidth filters. The PCS transmit (TX) band should have no more than −3.5 dB I.L. in-band (1850 to 1910 MHz in the U.S.) while having at least a 38.0 dB out-of-band rejection in the receive (RX) band (1930 to 1990 MHz range).

Further, this BPF must meet these specifications with a maximum constraint on height. A typical height constraint in present day handsets, for example, is 4.0 mm or less. To meet these demanding electrical requirements yet possess the smallest possible size and height, high order (>2^(nd) order) fixed-tuned filters constructed from either individual coaxial resonator elements or monoblock structures are usually necessary. In addition, to satisfy out-of-band rejection specifications, a transmission zero is usually required, increasing I.L. at the band edge. Because of variations in ceramics and fabrication tolerances, vendors must individually adjust the characteristics of fixed-tuned filters during their manufacture, driving costs higher.

Moreover, if more than one frequency band were to be supported (e.g., supporting the PCS bands in the U.S., Korea, and India) multiple fixed-tuned BPFs would be necessary, requiring extra switches which introduces additional loss. This is true, even if the power amplifier and low noise amplifier used have sufficient bandwidth to operate over these multiple bands.

A tunable BPF would allow the use of one BPF over several bands, or of a lower order filter to cover a bandwidth wider than a required passband at any particular time. To provide the tunability in a tunable BPF, a component capable of providing a variable capacitance is typically used.

Several structures are presently used to implement a variable capacitor. For example, movable parallel plates have been used for many years as the tuner in home radios. However, such plates are far too bulky, noisy, and impractical for use in most modern applications.

Another alternative, the electronic varactor, is a semiconductor device that adjusts capacitance responsive to an applied voltage. Because the varactor is typically noisy and lossy, particularly in applications above 500 MHz, it is ineffective for high-frequency, low-loss applications where high performance is required.

Another alternative, a micro-electro-mechanical-system (MEMS) is a miniature switching-device that may switch between capacitors responsive to an applied control signal. It, however, is costly, difficult to manufacture and of unproven reliability. In most cases, it provides discrete tuning, in that a system must select between a finite (and small) number of fixed capacitors.

Ferroelectric tunable capacitors are another alternative that has been attempted. Ferroelectric (f-e) materials are a class of materials, typically ceramic rare-earth oxides, whose prominent feature is that their dielectric constant (κ), and as a consequence, the electric permittivity (∈) changes in response to an applied slowly varying (DC or low frequency) electric field. The relationship of the dielectric constant (κ) and the electric permittivity (∈) of a material is given as follows: ∈=κ∈₀ where ∈₀ is the electric permittivity of a vacuum. At present, there are several hundred known materials that possess f-e properties. In a typical f-e material, one can obtain a range in κ by a factor of as much as approximately 3:1. The required DC voltage to generate such a change in κ depends on the dimensions of the f-e material over which a DC control voltage is applied. As a result of their variable dielectric constant, one can make tunable capacitors using f-e materials, because the capacitance of a capacitor depends on the dielectric constant of the dielectric proximate the capacitor conductors. Typically, a tunable f-e capacitor is realized as a parallel plate (overlay), interdigital (IDC), or a gap capacitor.

In known f-e variable capacitors, a layer of an appropriate f-e material, such as barium strontium titanate, Ba_(x)Sr_(1-x)TiO₃ (BSTO) is disposed adjacent to one or both conductors of a capacitor. Depending upon the strength of the electric field applied to the f-e material and the intrinsic properties of the f-e material selected, the capacitance changes. Typically, below the Curie temperature, T_(c), of the f-e film, the f-e material is in the ferroelectric state and will exhibit hysteresis in its response to a changing electric field. Above T_(c), f-e material is in the paraelectric state and will not exhibit hysteresis. Thus, one generally picks an f-e material whose T_(c) is lower than the expected operating temperature so as to operate in the paraelectric state, avoiding the hysteresis effects of the ferroelectric state.

However, conventional f-e variable capacitors have proven to be too lossy for use in insertion-loss-sensitive applications such as handsets. Moreover, these devices often perform unpredictably, preventing optimal design, construction, and use of f-e tunable filters.

Accordingly, there is a need in the art for improved tunable f-e filters capable of providing a tuning range over a desired frequency range with low I.L. and high out-of-band rejections and methods for designing the same.

SUMMARY

Fixed tuned bandpass filters must satisfy stringent size, insertion loss and out of band rejection, among other requirements. Tunable filters would be useful in replacing fixed tuned bandpass filters if they could meet these requirements. Lower order, or otherwise better, tunable filters might be used to tune over ranges requiring higher order fixed tuned filters. Or a single tunable filter could replace more than one fixed tuned filter. However, tunable filters require tunable components that have consistently shown themselves to be to high in insertion loss, unreliable, or possessing other prohibitive qualities.

It is desirable to provide a tunable bandpass filter that has superior insertion loss properties with respect to fixed-tuned bandpass filters yet still achieves required rejection performance and satisfies other requirements. It is therefore an object of this invention to provide tunable bandpass filters incorporating ferro-electric materials to tune the filters while maintaining a low insertion loss, meeting stringent out of band rejection requirements and satisfying other requirements. This is made possible by the advantageous design of capacitors and filters based on a correct recognition of the loss characteristics of the ferro-electric materials.

Another object of the invention is to provide a methodology for designing tunable bandpass filters. This methodology quantifies and minimizes loss mechanisms in tunable ferro-electric capacitors to select optimal structures for a tunable bandpass filter incorporating tunable ferro-electric capacitors.

The primary object of this process is to allow the user to design minimum loss BPF's that meet or exceed all other electrical and mechanical specifications placed on a conventional fix-tuned BPF that it replaces. The meeting or exceeding of performance specifications is critical if a tunable BPF is to replace a fix-tuned BPF in practical applications.

Proper f-e film characterization, along with optimum tunable BPF design procedures are mandatory if one is to achieve minimum loss tunable BPF's that simultaneously meet a stringent rejection specification.

In accordance with one embodiment of the invention, a method is provided for choosing a bandwidth and filter order for a tunable bandpass filter to satisfy an out-of-band rejection requirement and a passband insertion loss requirement. Given a topology for a ferro-electric capacitor, the method calculates the non-ferro-electric losses for the ferro-electric capacitor. Given a resonator having a first quality factor for coupling to the ferro-electric capacitor, the method determining the required ferro-electric loss of the f-e capacitor based upon the calculated non-ferro-electric losses and the first quality factor to achieve an insertion loss requirement for the tunable bandpass filter.

In accordance with another embodiment of the invention, a process is described by which a wide variety of f-e films can be efficiently and correctly characterized.

Further aspects and features of the invention are set forth in the following description together with the accompanying drawings.

BRIEF DESCRIPTION OF THE DRAWINGS

FIG. 1 a is a plan view of a ferro-electric gap capacitor.

FIG. 1 b is a cross-sectional view of the ferro-electric gap capacitor of FIG. 1 a taken along line A.

FIG. 2 a is a plan view of a ferro-electric overlay capacitor, along with an accompanying DC blocking capacitor.

FIG. 2 b is a plan view of the first metal layer in the overlay capacitor of FIG. 2 a.

FIG. 2 c is a cross-sectional view of the overlay capacitor of FIG. 2 a taken along line B in FIG. 2 a.

FIG. 3 illustrates an enlarged view of area C in FIG. 2 a.

FIG. 4 is a plan view of a ferro-electric interdigital capacitor.

FIG. 5 is a schematic of a resonator coupled to a tunable ferro-electric capacitor.

FIG. 6 is a schematic of a single pole tunable filter.

FIG. 7 is a planar circuit implementation of the single pole filter of FIG. 6

FIG. 8 a is a schematic of a double pole tunable filter having a ferro-electric capacitor configured to compensate for frequency response distortions induced by tuning.

FIG. 8 b is a schematic of a double pole tunable filter having a two ferro-electric capacitors configured to compensate for frequency response distortions induced by tuning.

FIG. 9 is a schematic of a divider network and direct current voltage source used to tune the two ferro-electric capacitors configured to compensate for frequency response distortions induced by tuning shown in FIG. 8 b.

FIG. 10 shows one implementation of the divider network shown in FIG. 9.

FIG. 11 a is a plan view of the tunable filter shown in FIG. 8 a.

FIG. 11 b is a cross-sectional view of the tunable filter shown in FIG. 11 a, taken along line D.

Use of the same reference symbols in different figures indicates similar or identical items.

DETAILED DESCRIPTION

In designing a tunable bandpass filter (BPF) for use and application in electronic signal processing systems, such as, for example, communications systems, one must usually meet or exceed both out-of-band rejection and pass band insertion loss (I.L.) requirements as well as size, weight and other mechanical, environmental and electrical requirements imposed on fix-tuned BPF's. Further, any such designs targeted for high volume products must be manufacturable and repeatable, with consistent unit-to-unit performance, requiring a minimum (and preferably no) added tuning or testing in-situ.

Thus, for a tunable BPF to be a commercially viable replacement for a fixed-tuned BPF, its performance should exceed that of the fixed-tuned BPF it is replacing in terms of most or all of the electrical and mechanical requirements. In demanding applications such as wireless handsets, passband I.L. must be minimized to prevent placing an even greater burden on other components in the handset. If a tunable BPF has I.L. greater than the fixed-tuned BPF it is to replace, the added I.L. may prove to be too great a burden on the overall system performance.

Many definitions of what defines a “pass band” may be used. Typically the pass band is defined by the points where the bandpass filter response falls to 3.0 dB below the mid-band, or band-center insertion loss (I.L₀.). However, any fixed filter response can be used to define the pass band. Higher order (more resonators) bandpass filters are typically required to meet a specific out-of-band rejection requirement. But increasing the filter order will increase the I.L₀. A useful basic relationship between filter order, topology and I.L₀. is given by the following equation: $\begin{matrix} {{I.L_{0}.} = {\left( {4.34*{Q_{1}/Q_{u}}} \right)*{\sum\limits_{i = 1}^{N}\quad g_{i}}}} & (1) \end{matrix}$ where N is the filter order,

Q_(u) is the unloaded Q of the resonators used,

Q_(l)=f₀/BW (BW is the 3 dB passband and f₀ is the midband frequency), and

g_(i) are the filter element values for a given topology (Chebyshev vs. Butterworth).

Generally, a Chebyshev response is preferable as it gives a steeper rejection response compared to that given by a Butterworth filter for a given filter order. Additionally, increasing the ripple in a Chebychev BPF further increases out of band rejection. As can be seen from equation (1), for a given filter order N, a larger passband results in lower I.L₀. as Q_(l) will decrease as BW increases. This lower I.L_(o). comes at the expense of decreased selectivity. To regain selectivity, the filter order N must be increased, at the expense of I.L₀. One of ordinary skill in the art of bandpass filter design will appreciate that equation (1) represents the best one can do for a given system requirement and filter order. Using a higher order filter (more resonators of a given unloaded Q) quickly increases I.L₀., because the g_(i) values get progressively larger in magnitude, even as there are more of them to sum (increased N). Note that equation (1) neglects implementation losses, which further increase I.L._(o), especially as the band edge is approached.

It can be seen from equation (1) that using a first or second order bandpass filter reduces I.L₀. At these lower orders, both the number (N) of the g_(i) coefficients decreases as well as the magnitudes of the g_(i). These low-order filters should be constructed from resonators that have the lowest loss (highest Q_(u)) so as to give the minimum I.L₀. possible. The resulting 1^(st) or 2^(nd) order bandpass filter will always have lower I.L₀. for a given resonator size and type (i.e., for a given Q_(u)) than the comparable fixed-tuned bandpass filter design of higher order. Tunability allows the low order narrowband BPF to replace a wider band, fix-tuned BPF. A tunable narrowband low order BPF can cover the entire band of interest, overcoming the limitation of having a narrow bandwidth. This assumes that the desired channel (information) bandwidth is narrower than the total system bandwidth.

Tunable BPFs have the best chance of replacing fixed-tuned BPFs in those cases where the fixed-tuned BPF covers a system bandwidth that is greater than that required for transmission or reception of a single channel. For example, a fixed-tuned BPF in a handset for operation in the U.S. CDMA PCS band covers such a BW. It will be understood that this is also true of U.S. cellular CDMA and many other standards. The techniques, methods and devices taught herein are applicable to many standards besides U.S. CDMA PCS. U.S. CDMA PCS is discussed as an example only.

In the full U.S. PCS band, 60 MHz is allocated for Tx (1850 to 1910 MHz) and 60 MHz for Rx (1930 to 1990 MHz) for full band operation. The CDMA standard is a full duplex system, meaning the handset must simultaneously transmit and receive. To accomplish this, a duplexer filter is needed to separate the bands and prevent interference. While the PCS band is 60 MHz wide, the individual CDMA channel is only 1.25 MHz wide. Current system architecture, however, forces CDMA PCS bandpass filters and multiplexers (including duplexers) to have a BW≧60 MHz as the system must allow for and accommodate operation of any 1.25 MHz channel in any region of the 60 MHz band.

A tunable PCS band filter could alter this situation by meeting the worst case rejection specifications while providing a lower order BPF of simpler topology that occupies a smaller physical area. Such a lower order filter would necessarily provide lower I.L₀. by virtue of equation (1). In some circumstances partial band operation, covering a band less than 60 MHz, is desired. Tunable BPF's would be equally advantageous in these circumstances.

To effectively replace a high-order fixed-tuned BPF with a low-order tunable BPF, three factors should be considered. First, the fractional bandwidth (i.e. Q_(l)) of the low-order BPF and the chosen topology must be such that the worst case rejection specification is met. Because Q_(l)=f₀/BW, as the 3 dB bandwidth (BW) decreases, the I.L. increases. Thus, if BW is too small relative to f₀, the resulting BPF will have an unacceptably high I.L., requiring a tradeoff between BW and I.L. For practical designs, a low-order tunable BPF should have the lowest possible I.L. consistent with meeting the worst-case required rejection. Some topologies are preferred in that they naturally provide a low side (below the transmission band) zero or a high side (above the transmission band) zero.

A topology such as that shown in FIG. 8 a, where the resonators 404 and 408 are electromagnetically coupled along their entire length, is one such topology. It produces a high or low side zero depending upon the capacitance of capacitor 432. This zero allows for a wider BW to be used, along with a BPF topology of lower ripple (resulting in numerically smaller g_(l) values), thus providing a lower I.L.₀ as seen in equation (1).

Second, the low-order tunable filter must be tunable to cover the entire BW, just as with a fixed-tuned filter. Finally, the tunable capacitor used within the low-order tunable filter should be of sufficiently low loss so the resulting filter has an I.L. that meets or exceeds specifications. Although a tunable 1^(st) or 2^(nd) order bandpass filter will be of minimum added loss compared to a higher order (N>2) fixed-tuned bandpass filter design, the tunable component (variable f-e capacitor) must have a fast tuning mechanism and be tunable to cover the entire bandpass range, using the available tuning voltage.

The total loss of a capacitor, L_(t), whether tunable or not, is given by a ratio of its dissipated to stored energy, where the energy is stored in the electric field and dissipated in resistance, i.e., L_(t)=(dissipated energy)/(stored energy). The inverse of this loss is the quality factor, Q=1/L_(t).

For a capacitor, L_(t) may be given by the quantity (ω*R_(s)*C), where ω is the frequency in radians, R_(s) is the total series resistance of the capacitor, and C is the capacitance. This definition of Q is valid for frequencies which are below self resonance due to the reactance of stray inductance associated with any real capacitor and above the frequency at which Rp effectively shunts C, that is, the capacitive reactance is much smaller than Rp. Over this range of frequencies, a real capacitor can be modeled as a resistance Rs in series with the desired capacitance. Thus, Q is inversely proportional to the quantity (ω*R_(s)*C). For example, as any of the quantities, C, ω and R_(s) is increased or decreased, all other factors being held constant, Q decreases or increases, respectively. Or, to keep Q constant, if one of the quantities, C, ω, or R_(s) is decreased or increased the product of the other two quantities must be increased or decreased, respectively.

The importance of determining the total loss given by an f-e capacitor in a resonant circuit can be seen from the following equations: L_(c)=1/Q_(c) and 1/Q_(T)=1/Q_(c)+1/Q_(u), where,

Lc=the loss of the capacitor;

Q_(T)=the total Q of the f-e capacitor and the resonator or inductor combined;

Q_(c)=the Q of the capacitor; and

Q_(u)=the Q of the unloaded resonator or alternatively, the Q of an inductor used to create a parallel resonant circuit.

As Q_(c) increases, it will affect the Q_(T) less and less. If Q_(c) is infinite, it has no affect on Q_(T). For practical purposes, this is also true if Q_(c) is approximately 10*Q_(u). The converse is true too. As Q_(u) becomes higher and higher relative to Q_(c), Q_(u) has less and less effect on Q_(T). In either case, the highest practical Q_(c) is desired.

For example, in the PCS band, for a 1.0 pF tunable capacitor to have a Q_(c)=250 at 2.0 GHz requires that R_(s) be 0.32Ω (ohms). This assumes Rp, the parallel resistance, which shunts C, is much greater than Zc, the impedance of the capacitor, at 2.0 GHz (where Rp>about 1.6 kΩ here, for example, as the absolute value of Zc=0.0126Ω), and that the capacitor self resonant frequency is well above 2.0 GHz, so that the series inductance is negligible. To minimize loss (obtain a low R_(s)), requires an accounting of all loss mechanisms present and an elimination of these loss mechanisms if possible.

For f-e devices, the total loss is governed by summing each source contribution as follows: L _(t) =L _(geom) +L _(attach) +L _(metal) +L _(sub) +L _(rad) +L _(meas) +L _(f-e);

where L_(geom) is derived from the topology of the capacitor,

L_(attach) is loss due to device attachment,

L_(metal) is the total metal loss,

L_(sub) is the base substrate loss (if present),

L_(rad) is the radiation loss, both desired and undesired,

L_(meas) is the total loss arising from measurement errors, and

L_(f-e) is the f-e loss tangent.

This loss allocation can first be used to obtain an accurate value of L_(f-e) (or f-e tan δ) at the desired operating frequency in the manner in which the f-e capacitor will be used. To correctly derive L_(f-e), one must eliminate or constrain all of the other loss contribution sources just described. For example, L_(geom) will vary according to topology, being best for an overlay capacitor, worse for a gap capacitor, and much worse for an IDC capacitor. Although this loss can be reduced and controlled, it is inherent to a device. Consequently, the choice of topology for a given f-e capacitor will affect the best possible Q_(c) attainable from the f-e capacitor. Electromagnetic (EM) software can establish a baseline loss for a desired geometry, assuming a lossless f-e film. This baseline loss represents the best (lowest) loss for a given geometry.

In general, a gap capacitor is easiest to fabricate. An IDC is next easiest, and an overlay capacitor is hardest of these three. Compared to an IDC, the gap capacitor will have a better Q but lower capacitance per unit cross section (W in FIG. 1 a). The IDC's capacitance is greater due to the use of a number of fingers per unit cross section. For many communication filter applications, however, large capacitance (C≧4.0 pF) is not needed. Thus, a gap capacitor often can provide adequate capacitance. The inherently high value of κ for most f-e films helps provide relatively high capacitance per unit cross section, W, compared to a conventional gap capacitor.

L_(attach) arises from discrete device attachment techniques, including, for example, solder, silver paint, or wire bonding. These attachment losses may be large and unpredictable. The lowest losses are achieved by direct fabrication of the f-e capacitor to the resonator or other RF circuitry, thus minimizing if not eliminating this loss component.

The inherent loss of a stand-alone f-e capacitor is of little consequence. What is of much greater consequence is any added loss arising from the attachment of the f-e capacitor to a circuit. Even if the f-e capacitor were lossless, should a large loss connection be used, the overall effect is that of a lossy f-e device. For example, if a Q≧250 at 2.0 GHz is desired for a capacitance of 1.0 pF, then the total series resistance R_(s) must be ≦0.32 ohm. Any additional loss will thus further reduce the Q of this capacitor. That this additional loss is external to the actual capacitor is irrelevant. Even unavoidable loss mechanisms, such as those due to mounting, for example, lower the effective Q of the capacitor from the perspective of its effect on the system.

For minimum added loss, the connection between the f-e capacitor and the resonator should provide the lowest added resistance. Thus, the electric currents and charges associated with the f-e capacitor should see a minimum added loss. Conventional bonding or mounting techniques, such as (but not limited to) soldering, wire bonding or silver paint or paste do not provide for such a low loss, controllable bond.

The added, unpredictable loss arising from the use of such bonding methods degrade the realized Q regardless of whether or not the f-e capacitor is being used for resonator tuning purposes or characterization of an f-e film. Thus, for best performance (lowest loss) the f-e capacitor structure should be directly fabricated onto or with the resonator it is meant to tune or onto other essential RF circuitry. Only by direct fabrication can there be a minimum loss transition for electromagnetic (EM) sources (currents) from the f-e tuning elements to the resonator. The desirable effects of direct f-e capacitor fabrication onto or with a resonator can be enhanced by the lack of sharp corners or transitions.

Factors for L_(metal) include the surface roughness (SR) of the metal, metal thickness as compared to skin depth, δs, and conductivity. SR may be effectively eliminated as a factor if SR is less than aproximately 10 micro inches root mean square (rms) for operating frequencies in the L and S band (1-4 GHz). The metal thickness may be reduced as a factor if the thickness is 1.5δs or greater, or effectively eliminated if the thickness is ≧5δs. For electrode contacts, metal thickness (t_(m)) can be approximately 1.5δs. For the case of electromagnetic resonators, where a travelling or standing wave must be supported, i.e., where the metal in question extends for an appreciable fraction of a wavelength (about 10% or greater), the metal thickness should be closer to about 5δs or greater.

Conductivity is best for silver, copper and gold (Ag, Cu, and Au, respectively). Thus, L_(metal) can be reduced and controlled, but not eliminated as a factor. Its effect, however, can be calculated by expressions well known to those skilled in the art, or by using line calculator tools available in commonly used circuit simulators, such as Eagleware or Touchstone. Further, precise fabrication control can bound geometric variations in L_(metal).

The loss contribution represented by L_(sub) may be minimized by choosing a low loss substrate with a loss tangent less than 0.001 and preferably less than 0.0005 at the operating frequency of interest. Suitable materials include >99% pure alumina, a best current choice for loss/cost benefits. Sapphire or MgO are better than alumina in that they have lower loss tangents, but they are more expensive. All these materials will accept f-e thin films without buffer layers and have a surface roughness that is acceptable with little or no further polishing. Semiconductor substrates are poor choices because of their relatively high conductivity. In addition to the factors of loss tangent, surface roughness and price, suitable substrates should not be brittle, can be fabricated as larger area wafers, and can be easily metallized without extensive pre-processing.

Separating out L_(sub) from the total loss of a composite substrate (f-e film plus substrate) can be achieved by using EM field or circuit simulation software. For example, Sonnet, Momentum, or IE3D may be used. Thus, L_(sub) can be reduced significantly and calculated precisely.

L_(rad) can be eliminated by proper shielding and design, and so is typically not a factor. It should be noted that a wide variety of filters, especially planar filters such as combline or hairpin, depend upon radiative coupling to achieve their desired performance. In these cases, one should ensure that the unwanted, stray coupling is reduced, if not eliminated.

L_(meas) can add significantly to the circuit loss error because small, added loss significantly reduces the measured Q of the device-under-test (DUT) or system thus obscuring the intrinsic Q of the DUT. The conventional method for measuring dielectric constant and loss tangent in a material is the cavity perturbation technique, which is well known to anyone skilled in the art. At L-band, however, the size of the cavity becomes quite large. When characterizing thin films (as opposed to bulk) with film thickness ≦1.5 μm, such as f-e films, the problem becomes very difficult as measurement errors can be severe. Furthermore, one should characterize an f-e capacitor (or filter) in a manner most similar to how it will be used. Thus, the preferred way to characterize f-e compounds or films is by microstrip resonator techniques.

For the purposes of determining f-e film characteristics and characterizing f-e capaictors, microstrip techniques are preferred to, for example, stripline or other volumetric techniques for f-e film characterization for the following reasons:

-   -   1) Microstrip circuits are planar systems with no substrate as a         top cover (which would be a stripline circuit), so no bonding of         hard substrates as top covers is required. So there is also no         need for continuity of ground planes (top to bottom) as needed         in a stripline, for example.     -   2) Preferably gap capacitors, and alternatively, IDC's, can be         readily fabricated and measured.     -   3) A large body of knowledge exists as to the characterization         of microstrip resonators.     -   4) No complex fixturing or fabrication or both are needed as are         required for dielectric cavities, for example.

One should measure high-Q circuits using resonator techniques because broadband measurement may not accurately resolve sub-ohm resistive losses at RF/microwave frequencies with any accuracy. For the same reason, LRC meters are not a good choice.

Measurement at radio frequency is requried to correctly obtain Q, and consequently Rs, for an f-e capacitor, since low frequency measurement, especially those below about 10 to 100 MHz, is dominated by a large parallel resistance, Rp, that shunts the capacitance in question. The dominance of Rp, along with the relatively small values of the capacitance in question (≦4.0 to 5.0 pF) prevents reliable Q (and therefore Rs) measurement at low frequencies.

When used to measure losses, wafer probe stations must be carefully used because it is difficult to calibrate out resistive and inductive loss at RF/microwave frequencies. Probe tips along with their ground connections are also sensitive to placement on the DUT as well as the pressure used to apply them. As a consequence, it is better to use a resonant test circuit that allows for direct measurement of the desired parameters in a way that does not require individual device loss measurements.

Thus, for measurements on resonant circuits, a network analyzer is the preferred choice. To minimize measurement loss and attain the most accurate measurement, one should calibrate out loss to the DUT, perform a full two port calibration of the network analyzer, and use averaging for calibration and measurement. Finally, proper analysis of the measured data, such as that outlined in “Data Reduction Method for Q Measurements of Strip-Line Resonators,” IEEE Transactions in MTT, S. Toncich and R. E. Collin, Vol. 40, No. 9, September 1992, pp. 1833-1836, hereby incorporated by reference, is required to accurately extract the Q, or loss, of the capacitor under test.

Using the results of above discussion to minimize, eliminate, or bound each of the foregoing losses, the total loss may be re-expressed as: L _(t) =L _(geom) +L _(metal) +L _(f-e) +ΔL _(misc)

As discussed above, both L_(geom) and L_(metal) may be quantified and removed analytically to obtain an accurate measure of L_(f-e). L_(geom) can be determined from an accurate electromagnetic simulation of the circuit based on a lossless f-e material assumption. L_(metal) can be determined using the expressions for metal loss assuming conductivity, SR (if applicable), and skin depth. The final term, ΔL_(misc), represents a combination of the incomplete removal of the other loss mechanisms or from the finite bounds on or incomplete removal of L_(metal) and L_(geom) or both. As such it represents an irreducible error term. For accurate measurements of f-e film/component properties, it should be minimized and bounded, as described in the preceding sections.

Finally, to reduce the effect of L_(f-e) to a minimum one must use selective f-e film deposition to place the f-e film only in regions where it is needed for tuning and nowhere else.

The process of accounting for all loss mechanisms and eliminating or bounding these losses not only determines f-e loss but also establishes correct design guidelines for low-loss tunable filters. Knowledge of L_(f-e) gives the designer a baseline for the f-e film that is necessary for doing any type of optimum design using f-e films. This knowledge is necessary if one is to effectively trade-off loss tangent for tunability, for example. In short, accurate fabrication and measurement techniques result in consistent f-e film loss characterization and application.

Given the above techniques for minimizing loss, preferred embodiments for the three types of f-e capacitors may now be discussed. It will be appreciated, that although these designs are for use in the L band (1-2 GHz), the teachings of the present invention may be used to design f-e capacitors for other frequency bands.

A preferred f-e tunable gap capacitor 10 is shown in FIGS. 1 a and 1 b for use in the cellular band (800 to 1000 MHz) and the L-band (1-2 GHz) for wireless handsets. The gap capacitor 10 is preferably formed on a ≧99% pure, 0.5 to 1.0 mm thick alumina, MgO, or sapphire substrate 12, having an SR less than a 5.0 micro inch RMS. Alternatively, the gap capacitor can be directly patterned on the front or rear face or a sidewall of any number of resonators structures. Examples are coaxial, monoblock or stripline resonators. Such a capacitor should be fabricated as close to its point of electrical connection to the resonator as possible.

The substrate 12 may have a metal ground plane 14 depending on other requirements. However, the preferred embodiment is without a ground plane to minimize stray capacitance. Preferably, a f-e layer 16 of approximately 0.1 to 2.0 microns in thickness formed of BSTO or other suitable or desirable f-e material for maximum capacitance and tuning range is deposited on the substrate 12. More preferably, layer 16 is 0.5 to 1.0 microns in thickness. The Ba/Sr fraction, doping, alloying, mixing with other components, and/or annealing determine the desired tuning characteristics and loss (tan δ), and therefore Q also.

Generally, it is preferred that the tuning characteristics meet the minimum required tuning range with the minimum tuning voltage. Preferably, x=0.5 in the Ba_(x)Sr_(1-x)TiO₃ composition for room temperature operation, regardless of doping with other elements and pre- or post-process annealing. It will be appreciated that other f-e materials beside BSTO may be used as well. A metal layer 18 formed on the f-e layer 16 defines a gap 20 that is preferentially 3.0 to 5.0 microns wide. Preferably, metal layer 18 is 0.5 to 6.0 microns thick. More preferably, metal layer 18 is 1.5 to 2.5 microns thick. It will be appreciated that the gap 20 can be wider or narrower than this range depending on requirements and processing equipment. For minimum added loss in the PCS band, the resulting capacitance will be approximately 0.6 pF to 1.5 pF at 0 volts DC while for the cellular CDMA band it will be about 1.0 pF to 3.0 pF. The width of the capacitor, W 17, will further determine the f-e capacitance, depending on the particular f-e film used and the desired gap 20. The width will typically be from 0.25 mm to 2.0 mm. The capacitance is typically 0.6 to 3.0 pF. The resulting capacitor should provide a Q of at least 80 at 2.0 GHz to meet the existing worst case CDMA PCS band BPF loss specification.

To minimize the added loss from the f-e film, selective deposition must be used, i.e., the f-e film is deposited only where needed for tuning and nowhere else as stated above. For example, in the gap capacitor 20 of FIG. 1 a, one could deposit the desired f-e film 16 in a narrow region D_(f-e) around the gap 20, as shown in FIG. 1 a. D_(f-e) should be large enough to ensure that the gap 20 can be repeatedly patterned over the f-e film in manufacturing (allowing for mask alignment tolerance) and to cover the needed area under the gap 20 for tuning purposes. For the L-band PCS filters, D_(f-e)=0.2 to 0.5 mm is adequate with 0.2 mm preferred. As the operating frequency increases D_(f-e) can decrease. As the operating frequency decreases, D_(f-e) can increase.

F-E film properties and fabrication will play a significant role in overall capacitor loss. Many techniques exist to mitigate and minimize f-e film loss. One feature of f-e films is that f-e film loss and tunability usually have an inverse relationship. That is, they usually must be traded off against each other. The greater the f-e κ tuning range, the greater the f-e loss in most cases.

Thus, even though f-e materials can achieve a κ tuning range of about 3 to 1, less tuning may be acceptable for a given filter application. In that case, less tuning would be chosen, with the benefit of less loss. For example, in the U.S. PCS CDMA band, the tuning requirement in the transmit band is from 1850 MHz to 1910 MHz, or about 4%. Thus, the f-e material can have significantly less tunability than 3 to 1.

For example, an f-e gap capacitor with 0.6 pF at 0V DC bias, needs to tune 33%, (from 0.6 pF down to 0.4 pF) to tune over the PCS transmit band. The actual tuning range depends on the BPF topology and the band over which the BPF must be tuned. The required tuning voltage to provide the 33% tuning in this example depends on the f-e capacitor geometry, including f-e film thickness, and the f-e film characteristics.

The effect of κ tunability on frequency tunability is determined by the filter topology. This effect must also be considered in choosing an f-e material. But without accurate characterization of the f-e loss to f-e κ tunability trade-off, a designer cannot even begin to choose an optimum f-e material. Accurate characterization of this trade-off allows a designer to choose an optimum f-e material (providing the lowest loss while meeting the tuning requirements).

With respect to L_(geom) for a gap capacitor, the major contributions to loss are the four corners formed by the gap. These losses can be reduced by rounding the corners.

In comparison to gap and interdigital capacitors, an overlay capacitor has the lowest L_(geom). An overlay capacitor is an example of a parallel plate geometry where the plate dimensions (length and width) are much greater than the plate separation. Given such a geometry, most of the electric field between the plates is uniform except for fringing along the edges. The fringing effect can be reduced significantly by the use of a guard band, as is well known in the art. Thus, the geometric loss from a parallel plate capacitor is quite low. In addition, parallel plate geometries can provide high capacitances along with high tuning from small control voltage swings.

A preferred overlay capacitor 30 is illustrated in FIGS. 2 a, 2 b, 2 c, and 3 that minimizes contributions to L_(geom). The capacitor 30 is deposited directly on a 25 mil alumina substrate 31. A first metal layer 34 bonds to the substrate 31. The shape of metal layer 34 is also illustrated in FIG. 2 b. A ferro-electric layer 36 overlies the metal layer 34. To form the overlay capacitor 30, a metal pad 40 formed on the ferro-electric layer 36 overlaps a portion of the first metal layer 34. FIG. 3 illustrates an enlarged view of the overlapping portions. Both the metal pad 40 and the metal layer 34 have a tapering region that forms an overlay capacitor 30 of the appropriate capacitance. An additional metal pad 41 overlaps the metal layer 34 to form a DC blocking capacitor 42. The metal pad 41 is tapered to form an appropriate capacitance for the DC blocking capacitor 42.

Due to the high dielectric constant (κ) of the most likely f-e films to be used, the overlay capacitor 30 may be quite small in area and still provide a capacitance (C_(f-e)) of 1.5 pF. A bonding bias pad 44 is provided for attachment of a high value (500-1000 kΩ) chip resistor. Note that the f-e film is deposited not only under the overlay capacitor 30 but also the blocking capacitor 42. However, the effect on the capacitance (C_(DC)) of the DC blocking capacitor 42 is irrelevant if C_(DC)≧180 pF and C_(f-e)≦1.5 pF, even under maximum V_(DC) bias (preferably 10V DC). This is because the DC blocking capacitor has a high enough capacitance that even when the capacitance is reduced by f-e tuning, it still has a minimal effect on C_(f-e).

In such an embodiment, 0.7≦C_(f-e)≦1.5 pF, f-e κ is approximately 1000, the overlapped portion of the metal pad 40 forming the overlap capacitor 30 is approximately 7.0 μm×7.0 μm, and the f-e film thickness is approximately 1.0 μm. The metal layer 34 may be Pt and have a thickness of ≦0.5 μm. The metal pads 40 and 41 may be Ag and have a thickness of approximately 1.5-2.5 μm.

While the L_(geom) of an overlay capacitor is lower than that of a gap capacitor, L_(f-e) of an overlay capacitor may be higher, as all of the rf field is concentrated in the f-e film. In a gap capacitor the rf field is partially in air, partially in the f-e film and partially in the substrate. For the same reasons, an overlay capacitor has greater capacitance tunability for a given applied voltage than a gap capacitor.

For a given cross sectional area, an IDC can provide a higher capacitance than a gap capacitor. It is more lossy, however, with the main contributions to L_(geom) including the gap spacing; loss increases as the gap spacing decreases. Similarly, loss increases as finger width decreases. The finger length also affects loss with loss increasing as finger length increases; especially in a microstrip (the most common) realization of an IDC as the odd mode loss dominates in such a structure. In addition, loss increases as the number of fingers increases due to loss introduced from the additional sharp corners; note that increasing the number of fingers is typically used to increase the capacitance of an IDC.

Many investigators in the f-e area have used IDC's with narrow finger widths and gaps (≦5.0 μm for each) to characterize f-e film. This is problematic, as such an IDC structure gives a high L_(geom) and therefore a low Q by itself. Typically, Q is much less than 100 at 2.0 GHz for about 1.0 pF, even without any L_(f-e). This makes it quite difficult to measure L_(f-e). The wide spread use of broad band measurement techniques, as described above, further obfuscates any L_(f-e) measurement.

A preferred IDC capacitor 60 is illustrated in FIG. 4 that minimizes the contributions to L_(geom). It is formed on a 99.5% pure alumina, MgO, sapphire or other suitable substrate 62 of thickness of approximately 0.2 to 1.5 mm. A f-e layer 64 is formed on the substrate 62. An input port 66 and output port 68 couple to the IDC capacitor 60. A metal layer 70 having a thickness of 1.5 to 3.0 microns and deposited on the f-e layer 64 forms a gap spacing 72 of approximately 5.0 microns and a finger width 70 of about 150 microns, or greater if possible.

A general methodology for constructing a tunable bandpass filter may now be described. As a first step, a designer must tradeoff the 3 dB bandwidth of the tunable filter with filter order to achieve the required out-of-band rejection. As is well known, as the filter order is increased, its rolloff rate increases, making it easier to achieve a required rejection specification. The rolloff is modeled as beginning at either of the 3 dB points defining the 3 dB bandwidth (BW). Thus, as the BW is decreased, it also becomes easier to achieve a required rejection specification.

For minimum loss the lowest order filter is desired. Typically, this will be a 2^(nd) order BPF. A low order BPF has a further advantage of being simpler to fabricate and tune, using fewer tunable resonators.

A Chebychev prototype BPF is preferred over a Butterworth as this gives the designer flexibility to trade off passband ripple with out-of-band rejection. The designer should strive to meet the worst case rejection specification by bandwidth adjustment without the addition of extra transmission zeros as transmission zeros increase filter complexity, cost and loss at the corresponding passband edge. One can, however, exploit topologies that have naturally occurring high or low side transmission zeros in this case.

Narrowing BW too much, however, will increase the insertion loss, as discussed above. Thus, the narrowest BW should be chosen that meets the required rejection specification over all specified operating conditions. If the chosen BW provides an unacceptable insertion loss, the BW should be increased, perhaps also requiring an increase in filter order or increased passband ripple (if acceptable). An additional high or low side transmission zero may be added if desired.

A tunable BPF requires control circuitry. This is an added expense, not required of fixed-tuned BPF's. Thus, a desirable tunable filter design should provide a decreased insertion loss, smaller size, or other benefit over that of a fixed-tuned BPF while meeting rejection specifications, to offset this expense. To achieve decreased insertion loss and smaller size, it is preferable to use no more than a one or two stage tunable filter. However, it will be appreciated that the principles of the invention may be advantageously used to design tunable f-e filters of arbitrary order.

Given a choice for filter order and BW that satisfies the rejection requirements, the highest possible Q_(u) for a resonator should be used to meet or exceed the required I.L., given size and height constraints. To define Q_(u), a topology should be chosen for the basic stage 100 illustrated in FIG. 5. Each stage 100 is formed by a resonator 102 coupled to a f-e capacitor 104. The f-e capacitor 104 may assume one of the forms described herein. The resonator 102 is shown as a grounded quarter wavelength resonator but an open circuit one-half wavelength resonator may also be used. Moreover, the resonator may be of other suitable electrical length.

The basic stage 100 may be considered a tunable EM resonator. The f-e capacitor 104 may be coupled either in series or in shunt with the resonator 102 as determined by the nature of their connection. As shown in FIG. 6, the f-e capacitor 104 is coupled in shunt with the resonator 102 such that Q_(f-e) of the f-e capacitor 104 affects the Q of the fix-tuned EM resonator 102. Volumetric resonators (e.g., coaxial, stripline, and monoblock) are preferred, as they provide the highest Q_(u) and smallest area and height at a minimal price compared to planar, i.e., microstrip or coplanar waveguide (CPW) alternatives.

Whether a tunable capacitor is placed in series or shunt with a volumetric resonator is often determined by the case of the connection; sometimes only one placement is even possible. Another key feature in determining whether a tunable capacitor is placed in series or shunt is that of minimum added loss and to a lesser extent, tuning range. A shunt connection will typically produce a more physically compact tunable filter than a series connection. It is usually easier to achieve as well. A series connection can provide better tuning in the case where electromagnetically coupled resonators (like monoblock, coaxial or stripline) are coupled along their entire extent (rather than coupled through a small aperture). A series connection is a more natural choice in these cases from a fabrication perspective.

As discussed above, the attachment losses may be significant if the f-e capacitor 104 is not integrated with the resonator 102 or other RF circuitry. Once a topology for the f-e capacitor 104 is chosen, its Q_(c) may be derived as discussed above. Q_(T) for the overall basic stage 100 is then given by 1/Q_(T)=1/Q_(c)+1/Q_(u).

where Q_(u) is the unloaded Q of the resonator 102;

and Qc is the Q of the f-e capacitor.

Given the Q_(T) for the basic stage 100, the designer may use equation (1) to determine if the required I.L. will be achieved or exceeded. Should the I.L. be too high, the designer may obtain a lower I.L. by increasing either or both of Q_(c) or Q_(u). If either Q_(c) or Q_(u) cannot be increased further, they will ultimately limit Q_(T). Further reduction of I.L._(o) can then be obtained only by switching to a lower loss topology. For example, Q_(u) may be increased if a volumetric instead of a microstrip resonator is used for a given footprint (area).

For high volume applications, such as CDMA wireless handsets, transverse electromagnetic (TEM) wave volumetric resonators are preferred. Such volumetric resonators can be either ceramic loaded coaxial resonators, slabline (monoblock) or stripline, to name the three most common realizations. The standard narrow band (typically defined as a BW≦10% of f_(o)) topology can be realized using top capacitively coupled (TCC) BPF's fabricated with either coaxial or stripline resonators. The TCC topology as shown in FIG. 8, lends itself to shunt f-e tuning, as this provides the most compact realization (having a smaller footprint than a TCC topology with series f-e tuning). Since grounded quarter wave resonators behave as parallel LC tuned circuits near resonance, placing an f-e tuning capacitor in shunt is advantageous.

Stepped impedance realizations of monoblock BPF's can be used as well. Monoblock resonators are typically EM coupled along their entire length, a direct consequence of their design. While they lend themselves to series f-e tuning, shunt tuning can be effectively used as well. Their electrical lengths can be tuned by the selective deposition and patterning of f-e tuning capacitors. Non-TEM resonators can be used as well, including, but not limited to, dielectric loaded waveguide resonators or dielectric pucks (with or without a shielded enclosure).

However, height restrictions may limit the achievable Q_(u) from volumetric resonators. An alternative to a volumetric coaxial resonator in such height-constrained systems is to use a stripline resonator. Here, one can make the center conductor wider (up to a point) thus improving Q_(u) while keeping the total height fixed. This embodiment has further merit in that the incorporation of a planar f-e capacitor such as a gap capacitor or IDC can be realized efficiently by making the top cover of the stripline resonator end before the location of the f-e capacitor. In this manner, the planar f-e capacitor would be formed on the portion of the substrate forming the bottom cover of the stripline resonator that extends beyond the top cover.

The formation of a “pedestal” on which the f-e capacitors can be optimally integrated as shown in FIG. 11 a for a TCC structure using coaxial resonators as an example. The f-e capacitors are integrated as extensions of the input and output capacitors 315 a and 315 b in FIG. 11 a on the pedestal. Alternatively, the f-e capacitors can be patterned and fabricated on the open ends (faces) (not shown) of the coaxial or monoblock resonators.

Regardless of the particular resonator being implemented, if height restrictions prevent any further increase in the Q_(u) of the resonator, Q_(c) would have to be increased instead by, for example, replacing an IDC f-e capacitor with a gap or an overlay f-e capacitor.

For many applications a single stage bandpass filter 140 will be satisfactory as illustrated in FIG. 6. As discussed with respect to FIG. 5, the bandpass filter 140 will include the f-e capacitor 104 and the resonator 102. A variable DC voltage 142 applied to the f-e capacitor 104 tunes the filter 140. The RF signal to be filtered is applied at input port 144 and is output at output port 146. Note that the input port 144 and output port 146 are interchangeable. A capacitor 143 is defined both between the input port 144 and the resonator 102. Another capacitor 145 is defined between the output port 146 and the resonator 102. The f-e capacitor 104, regardless of whether it is a gap, overlay, or IDC capacitor, is constructed to minimize losses in the manner described above. Similarly, the resonator 102, which may be either a shorted ¼ wavelength resonator or a ½ wavelength open circuit resonator, is selected to maximize Q_(u).

A higher Q_(u) will be provided by a volumetric resonator such as a coaxial resonator, a dielectric loaded waveguide, a monoblock, or a stripline resonator in a smaller footprint and at a lower cost. Alternatively, a larger area planar resonator such as a microstrip resonator may be used if specifications and price constraints permit. Most microstrip resonator circuits would be fabricated by thin film process on a hard substrate. As a result, they achieve less metal thickness than TEM resonators like coaxial and monoblock resonators that are metalized by thick film processes. Microstrip resonators are of larger size since part of the EM field is the air region above the microstrip.

Turning now to FIG. 7, a planar realization 150 of the bandpass filter 140 is illustrated. Resonator 102 is formed by a microstrip line 152 grounded through via 154. Note that microstrip line 152 could also be terminated in a suitable lossless ground plane (not illustrated), obviating the need for via 154. Capacitors 153 and 155 are formed by gaps between the input and output microstrip lines 156 and 158 and the resonator microstrip line 152. It is desirable to make the capacitance of capacitors 153 and 155 as large as practical (approximately 0.25 pF) to maximize input and output coupling while still maintaining a planar structure. The microstrip lines are formed on substrate 157 of 99.5% pure alumina, MgO, or sapphire that is preferably of thickness approximately 1.0 mm for providing a maximum microstrip resonator Q. The f-e capacitor 104 is formed as a gap capacitor by pad 160 and Mircrostrip line 152, with f-e layer 162 underneath pad 160 and microstrip line 152.

A variable DC voltage source biases pad 160 through resistor 164. A DC blocking capacitor is positioned between pads 160 and 166, where pad 166 includes a via 168 to ground. Note that pad 166 could also be terminated in a suitable lossless ground plane (not illustrated), obviating the need for via 168.

The DC blocking capacitor is needed if the resonator is shunted as shown in FIG. 7. The capacitance of the DC blocking capacitor is ideally at least 100 C_(f-e) to minimize its loading effects on C_(f-e). Its Q is ideally ≧40 in the band of interest. It will be appreciated that the choice of a gap capacitor and a microstrip resonator is arbitrary—any of the forms discussed herein could be employed consistent with the teachings of the present invention.

The bandpass filter of FIG. 7 may be ideally used as a test circuit to characterize an f-e film as described herein. As such, the bandpass filter of FIG. 7 provides the following advantages:

-   -   1) The f-e capacitor can be fabricated as it is to be used,         particularly if that realization is a gap capacitor or IDC.         Selective f-e deposition is used.     -   2) While an f-e gap capacitor is shown, an IDC could be used as         well. A gap capacitor has a simpler geometry. It is easier to         fabricate and has lower geometric loss compared to an IDC. It is         also easier to fabricate than an overlay capacitor.     -   3) Since the circuit is fabricated with thin film processing         techniques the geometry can be precisely controlled and         measured.     -   4) Metal thickness can be accurately measured by profilometry.         Metal type can be selected as desired (Au, Ag or Cu).     -   5) A high Q microstrip circuit completes the fixed resonator         part of the circuit.     -   6) The f-e capacitor is directly fabricated in the resonator.         There is no added loss due to soldering, bonding, etc. The         transition from resonator to f-e capacitor is uniform, or it can         be tapered, if desired.     -   7) No via holes are needed if large area ground planes and a         Wiltron test fixture (with jaws to hold and ground the circuit         top and bottom) is used. Drilling vias in hard substrates is a         significant cost adder and reduces the number of such test         circuits that can be fabricated.     -   8) This circuit can be accurately modeled in EM software.     -   9) This circuit can be fabricated without f-e film to determine         a base loss (at a higher f_(o), of course) of the circuit for         correlation to simulations.     -   10) The use of a low loss substrate minimizes its effect on the         overall circuit.     -   11) Measured results of f_(o) and I.L_(o). can be used to         extract f-e film dielectric constant and tan δ.     -   12) The circuit in FIG. 7 can be fabricated with an aperture in         the base substrate where the f-e cap is shown. Now, independent         f-e caps can be placed over the aperture, held in place with         pressure, allowing the f-e caps to be tested as stand-alone         components.

Referring now to FIG. 8 a, a two stage TCC tunable BPF 400 is illustrated. As discussed with respect to FIG. 5, each stage of bandpass filter 400 comprises a resonator 404 and 408 and f-e capacitor 410 a and 410 b. The resonators 404 and 408 are shown as ¼ wavelength short-circuited resonators but may also be ½ wavelength open circuit resonators. In either case, the resonator length is reduced by the presence of C_(f-e).

A variable DC voltage applied to the f-e capacitors 410 a and 410 b tunes the bandpass filter 400. The ferro-electric capacitors 410 a and 410 b couple to ground through DC blocking capacitors 412 a and 412 b, since the resonators are shorted in this example.

An RF signal is received at input port 402 and output at output port 406. Note that input port 402 and output port 406 are interchangeable. In addition to input capacitor 434 a and output capacitor 434 b, which are functionally similar to capacitors 143 and 145 discussed with respect to FIG. 6, an additional capacitor 432 is provided as an impedance or admittance inverter between the resonators 404 and 408 to create the desired BPF response. It will be appreciated that capacitor 432 can also be a discrete element or implemented through aperture coupling between resonators 404 and 408.

The tunable two-stage filters 400 and 450 illustrated in FIGS. 8 a and 8 b have a basic topology which creates a high or low side zero by the addition of electromagnetic coupling along the entire length of resonators 404 and 408. The zero can be used to provide better rejection for a given passband I.L. In the case of inter-resonator coupling along their entire length, the passband I.L. and out-of-band rejection will change as the ferro-electric capacitors tune the bandpass filter across the passband. To minimize any resulting distortion, particularly in the rejection band, capacitor 432 may be a f-e capacitor. Tuning capacitors 413 and 419 makes the zero track in frequency with the tunable passband.

To facilitate the biasing and tuning of f-e capacitor coupling between the resonators 404 and 408, capacitor 432 may be replaced by f-e capacitors 437 a and 437 b as shown in FIG. 8 b. Capacitors 437 a and 437 b ideally have a capacitance twice that of capacitor 432. In this embodiment, the ferro-electric capacitors 410 a, 410 b, 437 a and 437 b may all be tuned using a single DC tuning voltage VDC. Alternatively, different f-e materials can be deposited for capacitors 437 a and 437 b than that used for capacitors 410 a and 410 b. Thus greater versatility may be obtained in tuning with a single voltage.

The single DC tuning voltage for the f-e capacitors may be arranged as shown in FIG. 9. In FIG. 9, V_(DC) is coupled to a divider network 505. The divider network 505 is coupled to both f-e capacitors 437 a and 437 b. The divider network 505 is configured to provide the appropriate tuning range to the f-e capacitors 437 a and 437 b so as to cause the zero to track with the passband, as described above.

The divider network 505 may be constructed as shown in FIG. 10. In FIG. 10, V_(DC) is coupled to R₁. R₁ is coupled to R₂ and to both capacitors 437 a and 437 b. R₂ is also coupled to ground. R₁ and R₂ are chosen to cause the zero to track with the passband, as described above.

Alternatively, a separate voltage can be used to tune both capacitors 437 a and 437 b.

Turning now to FIG. 11 a, a tunable two-stage filter 300 using coaxial, monoblock resonators 302 a and 302 b is illustrated. Note that other resonator types could also be used. The resonators 302 a and 302 b may be open or short circuited. The resonators 302 a and 302 b attach to a first surface of a substrate 301. Pads 304 a and 304 b formed on the first surface of the substrate 301 couple to the resonators 302 a and 302 b through leads 305 a and 305 b. Pads 306 a and 306 b formed on the first surface of substrate 301 couple to pads 304 a and 304 b creating the desired gap for the ferro-electric capacitors 310 a and 310 b. Ferro-electric layers 312 a and 312 b underlying the pads 304 a and 304 b and 306 a and 306 b complete ferro-electric gap capacitors 310 a and 310 b. Note that the drawings are not to scale. Typically, the gap spacing is increased for clarity.

There are transmission lines 320 a and 320 b on a second surface of substrate 301. These transmission lines are used as input and output ports 320 a and 320 b for signals RF in and RF out. The input and output capacitors 315 a and 315 b are formed between the transmission lines 320 a and 320 b and the pads 304 a and 304 b with substrate 301 in between, as shown in FIG. 11 b. FIG. 11 b is a cross-sectional view of a portion of filter 300 shown in FIG. 11 a. The cross-section is taken along line B.

In addition, capacitor 321 is formed as a gap capacitor by the separation of pads 304 a and 304 b. Note that the coupling provided by capacitor 321 may alternatively be provided though aperture coupling between coaxial resonators 302 a and 302 b, eliminating the need for capacitor 321. It will be appreciated that although the coaxial resonators 302 a and 302 b are shown as separate structures, they may share a common wall to save space and permit any aperture coupling. Additionally, there may be no space and no wall between them. I.e., they may be mutually coupled monoblock resonators. In embodiments in which the coupling provided by capacitor 321 is implemented through aperture coupling, the pads 304 a and 304 b would be separated by a sufficient distance to minimize any gap capacitance between them. A bias voltage VDC couples through resistors 340 a and 340 b to tune the ferro-electric capacitors 310 a and 310 b. Each of the ferro-electric gap capacitors 310 a and 310 b couple to ground through DC blocking capacitors 341 a and 341 b.

Although the invention has been described with reference to particular embodiments, the description is only an example of the invention's application and should not be taken as a limitation. Consequently, various adaptations and combinations of features of the embodiments disclosed are within the scope of the invention as encompassed by the following claims. 

1. A tunable electromagnetic signal filter comprising: a dielectric constant adjustment signal generator for generating a dielectric constant adjustment signal; a first element having a capacitance; a second element having an inductance; the first and second elements configured as an electromagnetic signal filter having a resonant frequency; a ferro-electric material directly fabricated onto the first element for adjusting, responsive to the dielectric constant adjustment signal, the capacitance of the first element for adjusting the resonant frequency; wherein a quality factor of the first element, when operated in a temperature range between about −50 degrees Celsius and 100 degrees Celsius, is greater than about
 80. 2. The filter of claim 1, wherein the quality factor is greater than about
 180. 3. The filter of claim 1, wherein the quality factor is greater than about
 350. 4. A tunable electromagnetic signal filter comprising: a dielectric constant adjustment signal generator for generating a dielectric constant adjustment signal; an element having a capacitance and a quality factor; a volumetric resonator; the element and the resonator configured as an electromagnetic signal filter having a resonant frequency; a ferro-electric material directly fabricated onto the volumetric resonator for adjusting, responsive to the dielectric constant adjustment signal, the capacitance of the first element for adjusting the resonant frequency; and; wherein the tunable electromagnetic signal filter is constructed to operate in a temperature range between about −50 degrees Celsius and 100 degrees Celsius.
 5. The filter of claim 1 or 4, wherein the quality factor, when operated in a temperature range between about −50 degrees Celsius and 100 degrees Celsius, is greater than about 80 for a capacitance in a range between about 0.3 pF and 3.0 pF.
 6. The filter of claim 5, wherein the quality factor, when operated in a temperature range between about −50 degrees Celsius and 100 degrees Celsius, is greater than about 80 for a capacitance in a range between about 0.5 pF and 1.0 pF.
 7. The filter of claim 1 or 4 wherein the quality factor, when operated in a temperature range between about −50 degrees Celsius and 100 degrees Celsius, is greater than about 180 for a capacitance in a range between about 0.3 pF and3.0 pF.
 8. The filter of claim 7 wherein the quality factor, when operated in a temperature range between about −50 degrees Celsius and 100 degrees Celsius, is greater than about 180 for a capacitance in a range between about 0.5 pF and 1.0 pF.
 9. The filter of claim 1 or 4, wherein the resonator comprises a stripline resonator.
 10. The filter of claim 1 or 4, wherein the resonator comprises a monoblock resonator.
 11. The filter of claim 4, wherein a quality factor, when operated in a temperature range between about −50 degrees Celsius and 100 degrees Celsius, is greater than about
 80. 12. The filter of claim 4, wherein a quality factor, when operated in a temperature range between about −50 degrees Celsius and 100 degrees Celsius, is greater than about
 180. 13. A method of designing a tunable ferro-electric filter, the tunable ferro-electric filter having a resonant structure and constructed to operate in a tunable frequency range, comprising: generating a filter design for the filter, the filter design having a tunable device; determining a minimum acceptable efficiency for the tunable filter, the minimum acceptable efficiency being represented by a quality factor, Q, of about 80 or more; selecting a tunable ferro-electric device for use as the tunable device in the filter design; fabricating the ferro-electric device onto the resonant structure; and confirming that the Q is greater than about
 80. 14. The method of claim 13, wherein the Q is greater than about
 200. 15. The method of claim 13, wherein the Q is greater than about
 300. 